320 research outputs found

    Regularization of f(T)f(T) gravity theories and local Lorentz transformation

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    We regularized the field equations of f(T)f(T) gravity theories such that the effect of Local Lorentz Transformation (LLT), in the case of spherical symmetry, is removed. A "general tetrad field", with an arbitrary function of radial coordinate preserving spherical symmetry is provided. We split that tetrad field into two matrices; the first represents a LLT, which contains an arbitrary function, the second matrix represents a proper tetrad field which is a solution to the field equations of f(T)f(T) gravitational theory, (which are not invariant under LLT). This "general tetrad field" is then applied to the regularized field equations of f(T)f(T). We show that the effect of the arbitrary function which is involved in the LLT invariably disappears.Comment: 12 page

    On the Regularization of Kerr-NUT spacetime: I

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    Within the framework of teleparallel equivalent of general relativity (TEGR) theory, calculation of the total energy and momentum of Kerr-NUT spacetimes have been employed using two methods of the gravitational energy-momentum, which is coordinate independent, and the Riemannian connection 1-form, Γ~αβ{\widetilde{\Gamma}_\alpha}^\beta. It has been shown that the two methods give the same an unacceptable result, i.e., divergent value. Therefore, a local Lorentz transformation that plays a role of a regularizing tool, which subtracts the inertial effects without distorting the true gravitational contribution, has been suggested. This transformation keeps the resulting spacetime to be a solution of the equations of motion of TEGR.Comment: 10 pages, Latex (Will appear in Prog. Theor. Phys.

    Schwarzschild solution in extended teleparallel gravity

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    Tetrad field, with two unknown functions of radial coordinate and an angle Φ\Phi which is the polar angle ϕ\phi times a function of the redial coordinate, is applied to the field equation of modified theory of gravity. Exact vacuum solution is derived whose scalar torsion, T=TαμνSαμνT ={T^\alpha}_{\mu \nu} {S_\alpha}^{\mu \nu}, is constant. When the angle Φ\Phi coincides with the polar angle ϕ\phi, the derived solution will be a solution only for linear form of f(T)f(T) gravitational theory.Comment: 8 pages Late
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